SDO HMI 2014-04-03 02:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.87 | 61.13 | 16.40 | 45.74 | -7.98 | 7.60 | -48.85 | 95.01 | 0.7499 | 239.6 | 215.1 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.80 | -5.16 | 11.45 | -45.00 | 90.84 | 0.7067 | 608.0 | 547.1 | |
| 13.70 | 28.64 | 9.76 | 20.39 | -8.55 | 10.16 | -46.29 | 95.67 | 0.7207 | 883.2 | 551.1 | |
| 0.00 | 0.97 | 0.00 | 0.69 | -5.76 | 10.35 | -46.10 | 91.78 | 0.7196 | 510.0 | 363.0 | |
| 0.00 | 1.14 | 0.00 | 0.82 | -8.92 | 9.88 | -46.57 | 96.19 | 0.7240 | 290.0 | 305.5 | |
| 0.00 | 2.81 | 0.00 | 2.03 | -8.48 | 9.33 | -47.13 | 95.59 | 0.7306 | 487.0 | 420.2 | |
| 0.00 | 1.49 | 0.00 | 1.10 | -8.57 | 8.50 | -47.95 | 95.72 | 0.7403 | 362.0 | 325.1 | |
| 0.00 | 1.67 | 0.00 | 1.22 | -7.70 | 8.59 | -47.86 | 94.55 | 0.7394 | 618.0 | 508.6 | |
| 0.00 | 0.79 | 0.00 | 0.58 | -8.72 | 8.20 | -48.25 | 95.94 | 0.7438 | 605.0 | 519.2 | |
| 0.00 | 2.37 | 0.00 | 1.76 | -8.73 | 7.92 | -48.53 | 95.96 | 0.7469 | 507.0 | 423.0 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -8.54 | 7.86 | -48.59 | 95.71 | 0.7477 | 414.0 | 360.0 | |
| 0.00 | 0.61 | 0.00 | 0.49 | -7.67 | 4.44 | -52.01 | 94.69 | 0.7860 | -536.0 | -470.3 | |
| 8.17 | 16.43 | 6.64 | 13.35 | -7.29 | 3.56 | -52.89 | 94.26 | 0.7955 | -726.3 | -380.4 | |
| 0.00 | 0.79 | 0.00 | 0.65 | -6.91 | 3.32 | -53.13 | 93.79 | 0.7982 | -536.0 | -379.4 | |
| 0.00 | 2.02 | 0.00 | 1.66 | -6.98 | 3.10 | -53.35 | 93.89 | 0.8004 | -321.0 | -245.9 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |